arXiv · astro-ph/0411068
Large-scale inhomogeneities in modified Chaplygin gas cosmologies
Abstract
We extend the homogeneous modified Chaplygin cosmologies to large-scale perturbations by formulating a Zeldovich-like approximation. We show that the model interpolates between an epoch with a soft equation of state and a de Sitter phase, and that in the intermediate regime its matter content is simply the sum of dust and a cosmological constant. We then study how the large-scale inhomogeneities evolve and compare the results with cold dark matter (CDM), $Λ$CDM and generalized Chaplygin scenarios. Interestingly, we find that unlike the latter, our models do always resemble $Λ$CDM.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Luis P. Chimento, Ruth Lazkoz. 2005-05-18. Large-scale inhomogeneities in modified Chaplygin gas cosmologies. https://doi.org/10.1016/j.physletb.2005.04.029
Cite the original work for its findings. Save a collection to share your selection of sources.